Geometric actions and flat space holography

Dec 17, 2019
61 pages
Published in:
  • JHEP 02 (2020) 125
  • Published: Feb 21, 2020
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Abstract: (Springer)
In this paper we perform the Hamiltonian reduction of the action for three- dimensional Einstein gravity with vanishing cosmological constant using the Chern-Simons formulation and Bondi-van der Burg-Metzner-Sachs (BMS) boundary conditions. An equivalent formulation of the boundary action is the geometric action on BMS3_{3} coad- joint orbits, where the orbit representative is identified as the bulk holonomy. We use this reduced action to compute one-loop contributions to the torus partition function of all BMS3_{3} descendants of Minkowski spacetime and cosmological solutions in flat space. We then consider Wilson lines in the ISO(2, 1) Chern-Simons theory with endpoints on the boundary, whose reduction to the boundary theory gives a bilocal operator. We use the expectation values and two-point correlation functions of these bilocal operators to compute quantum contributions to the entanglement entropy of a single interval for BMS3_{3} invariant field theories and BMS3 blocks, respectively. While semi-classically the BMS3_{3} boundary theory has central charges c1_{1} = 0 and c2_{2} = 3/GN_{N}, we find that quantum corrections in flat space do not renormalize GN_{N}, but rather lead to a non-zero c1_{1}.
Note:
  • 61 pages, v2: typo's fixed and ref's added, v3: added comments and improved discussions. Matches version accepted for publication in JHEP
  • Gauge-gravity correspondence
  • Chern-Simons Theories
  • Field Theories in Lower Dimensions
  • Conformal and W Symmetry
  • partition function: torus
  • cosmological constant: 0
  • space-time: Minkowski
  • entropy: entanglement
  • correction: quantum
  • dimension: 3